Nonimaging optical illumination system

ABSTRACT

A nonimaging illumination optical device for producing a selected far field illuminance over an angular range. The optical device includes a light source 102, a light reflecting surface 108, and a family of light edge rays defined along a reference line 104 with the reflecting surface 108 defined in terms of the reference line 104 as a parametric function R(t) where t is a scalar parameter position and R(t)=k(t)+Du(t) where k(t) is a parameterization of the reference line 104, and D is a distance from a point on the reference line 104 to the reflection surface 108 along the desired edge ray through the point.

Certain rights in this invention are retained by the U.S. Government pursuant to contract DE FG02-87ER 13726 of the U.S. Department of Energy.

Continuation of prior application Ser. No. 08/745,239, filed Nov. 8, 1996, now U.S. Pat. No. 5,816,693 which is a continuation of U.S. Ser. No. 08/054,816, filed Apr. 28, 1993 now U.S. Pat. No. 5,586,013.

The present invention is directed generally to a method and apparatus for providing user selected nonimaging optical outputs from various types of electromagnetic energy sources. More particularly, the invention is directed to a method and apparatus wherein the design profile of an optical apparatus for extended optical sources can be determined by controlling the shape of the reflector surface to a family of edge rays while simultaneously controlling the full contour of the reflected source. By permitting such a functional dependence, the nonimaging output can be well controlled using various different types of light sources.

Methods and apparatus concerning illumination by light sources are set forth in a number of U.S. patents including, for example, U.S. Pat. Nos. 3,957,031; 4,240,692; 4,359,265; 4,387,961; 4,483,007; 4,114,592; 4,130,107; 4,237,332; 4,230,095; 3,923,381; 4,002,499; 4,045,246; 4,912,614 and 4,003,638 all of which are incorporated by reference herein. In one of these patents the nonimaging illumination performance was enhanced by requiring the optical design to have the reflector constrained to begin on the emitting surface of the optical source. However, in practice such a design was impractical to implement due to the very high temperatures developed by optical sources, such as infrared lamps, and because of the thick protective layers or glass envelopes required on the optical source. In other designs it is required that the optical reflector be separated substantial distances from the optical source. In addition, when the optical source is small compared to other parameters of the problem, the prior art methods which use the approach designed for finite size sources provide a nonimaging output which is not well controlled; and this results in less than ideal illumination. Substantial difficulties arise when a particular illumination output is sought but cannot be achieved due to limitations in optical design. These designs are currently constrained by the teachings of the prior art that one cannot utilize certain light sources to produce particular selectable illumination output over angle.

It is therefore an object of the invention to provide an improved method and apparatus for producing a user selected nonimaging optical output from any one of a number of different light sources.

It is another object of the invention to provide a novel method and apparatus for providing user selected nonimaging optical output of light energy from optical designs by controlling edge rays of a reflected fight source.

It is a further object of the invention to provide an improved optical apparatus and method of design wherein the reflector surface is tailored to a family of edge rays.

It is a further object of the invention to provide an improved optical apparatus and method of design for radiation collection.

It is yet another object of the invention to provide a novel optical device and method for producing a user selected intensity output by simultaneously controlling the full contour of a reflected source and taioring the reflector to a family of edge rays.

It is still an additional object of the invention to provide an improved method and apparatus for providing a nonimaging optical illumination system which generates a substantially uniform optical output over a wide range of output angles for finite size light sources.

Other objects, features and advantages of the present invention will be apparent from the following description of the preferred embodiments thereof, taken in conjunction with the accompanying drawings described below wherein like elements have like numerals throughout the several views.

DESCRIPTION OF THE DRAWINGS

FIG. 1 shows a two-dimensional optical device for providing nonimaging output;

FIG. 2 illustrates a portion of the optical device of FIG. 1 associated with the optical source and immediate reflecting surface of the device.

FIG. 3A illustrates a bottom portion of an optical system and FIG. 3B shows the involute portion of the reflecting surface with selected critical design dimensions and angular design parameters associated with the source;

FIG. 4A shows a perspective view of a three-dimensional optical system for nonimaging illumination and FIG. 4B illustrates a portion of the optical system of FIG. 4A;

FIG. 5A shows intensity contours for an embodiment of the invention and FIG. 5B illustrates nonimaging intensity output contours from a prior art optical design;

FIG. 6A shows a schematic of a two dimensional Lambertian source giving a cos³ θ illuminance distribution; FIG. 6B shows a planar light source with the Lambertian source of FIG. 6A; FIG. 6C illustrates the geometry of a nonimaging reflector providing uniform illuminance to θ=40° for the source of FIG. 6A; and FIG. 6D illustrates a three dimensional Lambertian source giving a cos⁴ θ illuminance distribution;

FIG. 7A shows a two dimensional solution ray trace analysis and FIG. 7B illustrates three empirical fits to the three dimensional solution;

FIG. 8 shows an acceptance angle function which produces a constant irradiance on a distant plane from a narrow one-sided lambertian strip source (2D) with a=1;

FIG. 9 illustrates a reflector profile which produces a constant irradiance on a distant plane from a one-sided lambertian strip source (2D) at the origin, R(φ=π/2)=1, a=1. CEC (inner curve) and CHC-type solutions (outer truncated curve) are shown;

FIG. 10 shows a reflector designed to produce a reflected image adjacent to the source; the combined intensity radiated in the direction -θ is determined by the separation of the two edge rays: R sin 2α;

FIG. 11 illustrates an acceptance angle function which produces a constant irradiance on a distant plane from a finite one-sided lambertian strip source; there is only a CHC-type solution;

FIG. 12 shows a reflector profile which produces a constant irradiance on a distant plane from a finite one-side larnbertian strip source of width two units; note that there is only a CHC-type solution and it is truncated;

FIG. 13 illustrates a deviation of the reflector depicted in FIG. 12 from a true V-trough;

FIG. 14 shows a desired irradiance distribution on a distant plane perpendicular to the optical plane divided by the irradiance produced along the axis by the source alone; a broken line shows the irradiance of a truncated device;

FIG. 15 illustrates an angular power distribution corresponding to the irradiance distribution shown in FIG. 13; a broken line refers to a truncated device;

FIG. 16 shows an acceptance angle function corresponding to the desired irradiance distribution plotted in FIG. 13;

FIG. 17 illustrates a reflector profile which produces the desired irradiance shown in FIG. 13 on a distant plane from a finite one-sided lambertian strip source of width two units; note that there is only a CHC-type solution and it is truncated;

FIG. 18 shows the slope of the refector as a function of vertical distance from the source;

FIG. 19 illustrates the deviation of the reflector depicted in FIG. 16 from a true V-trough;

FIG. 20 shows the effect of truncation indicated by the angle up to which the truncated device matches the desired power distribution, and plotted as a function of the vertical length of the reflector,

FIG. 21 illustrates a light source and family of edge rays given along a reference line with identifying vectors;

FIG. 22A illustrates a source, reflector, reference line and edge rays for a CEC reflector and FIG. 22B is for a CHC reflector;

FIG. 23 illustrates the effect of termination of the reflector on boundary illumination;

FIG. 24 shows a reflector for illumination of both sides of a target zone;

FIG. 25 shows irradiance as a function of angle on a distant plane from a finite cylindrical source of uniform brightness;

FIG. 26 shows a CEC-type reflector profile producing a constant irradiance on a distant plane from a cylindrical source; and

FIG. 27 shows some edge rays corresponding to the angles designated in FIG. 25.

DETAILED DESCRIPTION OF PREFERRED EMBODIMENTS A. Small Optical Sources

In the design of optical systems for providing nonimaging illuniination using optical sources which are small relative to other system parameters, one should consider the limiting case where the source has no extent. That is, for example, the size of the source is much less than the closest distance of approach to any reflective or refractive component. Thus the angle subtended by the source at any reflective or refractive component may be regarded as small. Our approximation of small source dimension d and large observer distance D amounts to d<<R₀ <<D. This is in a sense the opposite of the usual nonimaging problem where the finite size and specific shape of the source is critical in determining the desizn. In any practical situation, a source of finite, but small, extent can better be accomodated by the small-source nonimaging design described herein rather than by the existing prior art finite-source designs.

We can idealize a source by a line or point with negligible diameter and seek a one-reflection solution in analogy with the conventional "edge-ray methods" of nonimaging optics (see, for example, W. T. Welford and R. Wnston "High Collection Nonimazing Optics," Academic Press New York, N.Y. (1989)). Polar coordinates R, Φ are used with the source as origin and θ for the angle of the reflected ray as shown in FIG. 3. The geometry in FIG. 3 shows that the following relation between source angle and reflected angle applies:

    d/dΦ(logR)=tan α,                                (1)

where α is the angle of incidence with respect to the normal.

Therefore,

    α=(Φ-θ)/2                                  (2)

Equation (1) is readily integrated to yield,

    log(R)=∫tan αdΦ+const.                      (3)

so that,

    R=const. exp ∫(tan αdΦ)                     (4)

This equation (4) determines the reflector profile R(Φ) for any desired functional dependence θ(Φ).

Suppose we wish to radiate power (P) with a particular angular distribution P(θ) from a line source which we assume to be axially symmetric. For example, P(θ)=const. from θ=0 to θ₁ and P(θ) ˜0 outside this angular range. By conservation of energy P(θ)dΦ=P(Φ)dΦ (neglecting mraterial reflection loss) we need only ensure that

    dθdΦ=P(Φ)/P(θ)                         (5)

to obtain the desire radiated beam profile. To illustrate the method, consider the above example of a constant P(θ) for a fine source. By rotational symmetry of the line source, dP/dΦ=a constant so that, according to Equation (4) we want θ to be a linear function of Φ such as, θ=aΦ. Then the solution of Equation (3) is

    R=R.sub.0 /cos.sup.k (Φ/k)                             (6)

where,

    k=2/(1-a),                                                 (7)

and R₀ is the value of R at Φ=0.

We note that the case a=0(k=2) gives the parabola in polar form,

    R=R.sub.0 /cos.sup.2 (Φ/2),                            (8)

while the case θ=constant=θ₁ gives the off-axis parabola,

    R=R.sub.0 cos.sup.2 (θ.sub.1 /2)/cos.sup.2 [Φ-θ.sub.0)/2](9)

Suppose we desire instead to illuminate a plane with a particular intensity distribution. Then we correlate position on the plane with angle q and proceed as above. Turning next to a spherically symmetric point source, we consider the case of a constant P(Ω) where Ω is the radiated sold angle. Now we have by energy conservation,

    P(Ω)dΩ=P(Ω.sub.0)dΩ.sub.0          (10)

where Ω₀ is the solid angle radiated by the source. By spherical symmetry of the point source, P(Ω₀)=constant. Moreover, we have dΩ=(2π)dcosθ and dΩ₀ =(2π)dcosΦ; therefore, we need to make cosθ a linear function of cosΦ,

    cosθ=a cos Φ+b                                   (11).sub.1

With the boundary conditions that θ=0 at Φ=θ, θ=θ₁ at Φ=Φ₀, we obtain,

    a=(1-cosθ.sub.1)/(1-cosΦ.sub.0)                  (12)

    b=(cosθ.sub.1 -cosΦ.sub.0)/(1-cosΦ.sub.0)    (13)

[For example, for θ₁ <<1 and Φ₀ ˜π/2 we have, θ˜√2θ₀ sin(1/2Φ).] This functional dependence is applied to Equation (4) which is then integrated, such as by conventional numerical methods.

A useful way to describe the reflector profile R(Φ) is in terms of the envelope (or caustic) of the reflected rays r(Φ). This is most simply given in terms of the direction of the reflected ray t=(-sinθ, cosθ). Since r(Φ) lies along a reflected ray, it has the form,

    r=R+Lt.                                                    (14)

where R=R(sinΦ₁ -cosΦ). Moreover,

    RdΦ=Ldθ                                          (15)

which is a consequence of the law of reflection. Therefore,

    r=R+Rt/dθ/dφ                                     (16)

In the previously cited case where θ is the linear function aΦ, the caustic curve is particularly simple,

    r=R+t/a                                                    (17)

In terms of the caustic, we may view the reflector profile R as the locus of a taut string; the string unwraps from the caustic r while one end is fixed at the origin.

In any practical design the small but finite size of the source will smear by a small amount the "point-like" or "line-like" angular distributions derived above. To prevent radiation from returning to the source, one may wish to "begin" the solution in the vicinity of θ=0 with an involute to a virtual source. Thus, the reflector design should be involute to the "ice cream cone" virtual source. It is well known in the art how to execute this result (see, for example, R. Wmston, "Appl. Optics," Vol. 17, p. 166 (1978)). Also, see U.S. Pat. No. 4,230,095 which is incorporated by reference herein. Similarly, the finite size of the source may be better accommodated by considering rays from the source to originate not from the center but from the periphery in the manner of the "edge rays" of nonimaging designs. This method can be implemented and a profile calculated using the computer program of the Appendix (and see FIG. 2) and an example of a line source and profile is illustrated in FIG. 1. Also, in case the beam pattern and/or source is not rotationally symmetric, one can use crossed two-dimensional reflectors in analogy with conventional crossed parabolic shaped reflecting surfaces. In any case, the present methods are most useful when the sources are small compared to the other parameters of the problem.

Various practical optical sources can include a long arc source which can be approximated by an axially symmetric line source. We then can utilize the reflector profile R(φ) determined hereinbefore as explained in expressions (5) to (9) and the accompanying text. This analysis applies equally to two and three dimensional reflecting surface profiles of the optical device.

Another practical optical source is a short arc source which can be approximated by a spherically symmetric point source. The details of determining the optical profile are shown in Equations (10) through (13).

A preferred form of nonimaging optical system 20 is shown in FIG. 4A with a representative nonimaging output illustrated in FIG. 5A. Such an output can typically be obtained using conventional infrared optical sources 22 (see FIG. 4A), for example high intensity arc lamps or graphite glow bars. Reflecting side walls 24 and 26 collect the infrared radiation emitted from the optical source 22 and reflect the radiation into the optical far field from the reflecting side walls 24 and 26. An ideal infrared generator concentrates the radiation from the optical source 22 within a particular angular range (typically a cone of about [%]15 degrees) or in an asymmetric field of [%]20 degrees in the horizontal plane by a [%]6 degrees in the vertical plane. As shown from the contours of FIG. 5B, the prior art paraboloidal reflector systems (not shown) provide a nonuniform intensity output, whereas the optical system 20 provides a substantially uniform intensity output as shown in FIG. 5A. Note the excellent improvement in intensity profile from the prior art compound parabolic concentrator (CPC) design. The improvements are summarized in tabular form in Table I below:

                  TABLE I                                                          ______________________________________                                         Comparison of CPC with Improved Design                                                              CPC  New Design                                           ______________________________________                                         Ratio of Peak to On Axis Radiant Intensity                                                            1.58   1.09                                             Ratio of Azimuth Edge to On Axis                                                                      0.70   0.68                                             Ratio of Elevation Edge to On Axis                                                                    0.63   0.87                                             Ratio of Corner to On Axis                                                                            0.33   0.52                                             Percent of Radiation Inside Useful Angles                                                             0.80   0.78                                             Normalized Mouth Area  1.00   1.02                                             ______________________________________                                    

In a prefered embodiment designing an actual optical profile involves specification of four parameters. For example, in the case of a concentrator design, these parameters are:

1. a=the radius of a circular absorber;

2. b=the size of the gap;

3. c=the constant of proportionality between θ and Φ-Φ₀ in the equation θ=_(c) (Φ-Φ₀);

4. h=the maximum height.

A computer program has been used to carry out the calculations, and these values are obtained from the user (see lines six and thirteen of the program which is attached as a computer sofware Appendix included as part of the specification).

From Φ=0 to φ=Φ₀ in FIG. 3B the reflector profile is an involute of a circle with its distance of closest approach equal to b. The parametric equations for this curve are parameterized by the angle α (see FIG. 3A). As can be seen in FIG. 3B, as Φ varies from 0 to Φ₀, α varies from α₀ to ninety degrees. The angle α₀ depends on a and b, and is calculated in line fourteen of the computer software program. Between lines fifteen and one hundred and one, fifty points of the involute are calculated in polar coordinates by stepping through these parametric equations. The (r,θ) points are read to arrays r(i), and theta(i), respectively.

For values of Φ greater than Φ₀, the profile is the solution to the differential equation:

    d(lnr)/dΦ=tan{1/2[Φ-θ+arc sin(a/r]}

where θ is a function of φ. This makes the profile r(φ) a functional of θ. In the sample calculation performed, θ is taken to be a linear function of Φ as in step 4. Other functional forms are described in the specification. It is desired to obtain one hundred fifty (r,theta) points in this region. In addition, the profile must be truncated to have the maximum height, h. We do not know the (r,theta) point which corresponds to this height, and thus, we must solve the above equation by increasing phi beyond Φ₀ until the maximum height condition is met. This is carried out using the conventional fourth order Runga-Kutta numerical integration method between lines one hundred two and one hundred and fifteen. The maximum height condition is checked between lines one hundred sixteen and one hundred twenty.

Once the (r,theta) point at the maximum height is known, we can set our step sizes to calculate exactly one hundred fifty (r,theta) points between φ₀ and the point of maximum height. This is done between lines two hundred one and three hundred using the same numerical integration procedure. Again, the points are read into arrays r(i), theta(i).

In the end, we are left with two arrays: r(i) and theta(i), each with two hundred components specifying two hundred (r,theta) points of the reflector surface. These arrays can then be used for design specifications, and ray trace applications.

In the case of a uniform beam design profile, (P(θ)=constant), a typical set of parameters is (also see FIG. 1):

a=0.055 in.

b=0.100 in.

h=12.36 in.

c=0.05136

for θ(Φ)=c(Φ-Φ₀)

In the case of an exponential beam profile (P(θ)=ce^(-a)θ) a typical set of parameters is: ##EQU1##

Power can be radiated with a particular angular distribution P^(o) (θ) from a source which itself radiates with a power distribution P^(o) (φ). The angular characteristic of the source is the combined result of its shape, surface brightness, and surface angular enissiviry at each point. A distant observer viewing the source fitted with the reflector under an angle θ will see a reflected image of the source in addition to the source itself. This image will be magnified by some factor [M] if the reflector is curved. Ideally both the source and its reflected image have the same brightness, so the power each produces is proportional to the apparent size. The intensity perceived by the observer, P^(o) (θ) will be the sum of the two

    P.sup.o (θ)=P.sup.o (θ)+|M|P.sup.o (θ).(18)

The absolute value of the magnification has to be taken because, if the reflected image and the source are on different sides of the reflector and we therefore perceive the image as reversed or upside down, then the magnification is negative. Actually, at small angles, the source and its reflection image can be aligned so that the observer perceives only the larger of the two. But if [M] is large, one can neglect the direct radiation from the source.

Thus, one is concerned with the magnification of the reflector. A distant observer will see a thin source placed in the axis of a trough reflector magnified in width by a factor ##EQU2##

This can be proved from energy conservation since the power emitted by the source is conserved upon reflection: P^(S) dφ=M P^(S) dθ.

For a rotationally symmetric reflector the magnification, Mm as given in Eq.(19) refers to the meridional direction. In the sagittal direction the magnification is ##EQU3## where now μ₁ and μ₂ are small angles in the sagittal plane, perpendicular to the cross section shown in FIG. 2. Equation (20) can be easily verified by noting that the sagittal image of an object on the optical axis must also lie on the optical axis. The reason for this is that because of symmetry, all reflected rays must be coplanar with the optical axis.

The total magnification M_(t) is the product of the sagittal and the meridional magnification ##EQU4##

Actually Eq.(21) could also have been derived directly from energy conservation by noting that the differential solid angle is proportional to d cos(θ) and d cos(φ) respectively.

Thus, inserting the magnification given in Eq. (21) or Eq.(19), as the case may be, into Eq.(18) yields the relationship between φ and θ which produces a desired power distribution P(θ) for a given angular power distribution of the source P^(S). This relationship then can be integrated as outlined in Eq. 17 to construct the shape of the reflector which solves that particular problem.

There are two qualitatively different solutions depending on whether we assume the magnification to be positive or negative. If Mm>0 this leads to CEC-type devices, whereas Mm<0 leads to CHC-type devices. The term CEC refers to Compound Elliptical Concentrator and CHC to the so called Compound Hyperbolic Concentrator.

Now the question arises of how long we can extend the reflector or over what angular range we can specify the power distribution. From Eq.(17) one can see that if φ-θ=π then R diverges. In the case of negative magnification this happens when the total power seen by the observer between θ=0 and θ=θ^(max) approaches the total power radiated by the source between φ=0 and φ=π. A similar limit applies to the opposite side and specifies θ^(min). The reflector asymptotically approaches an infinite cone or V-trough. There is no power radiated or reflected outside the range θ^(min) <θ<θ^(max).

For positive magnification the reflected image is on the opposite side of the symmetry axis (plane) to the observer. In this case the limit of the reflector is reached as the reflector on the side of the observer starts to block the source and its reflection image. For symmetric devices this happens when φ+θ=π. In this case too one can show that the limit is actually imposed by the first law. However, the reflector remains finite in this limit. It always ends with a vertical tangent. For symmetric devices where θ^(max) =-θ^(min) and φ^(max) =φ^(min) the extreme directions for both the CEC-type and the CHC-type solution are related by

    φ.sup.max +θ.sup.max =π                       (22)

In general CEC-type devices tend to be more compact. The mirror area needed to reflect a certain beam of light is proportional to 1/cos(α). The functional dependence of θ and φ for syntnetrical problems is similar except that they have opposite signs for CHC-type devices and equal signs for CEC-type solutions. Therefore α increases much more rapidly for the CHC-type solution which therefore requires a larger reflector, assuming the same initial value R₀. This is visualized in FIG. 8 and where the acceptance angle function as well as the incidence angle α are both plotted for the negative magnification solution.

To illustrate rate the above principles, consider a strip source as an example. For a narrow, one-sided larnbertain strip, the radiant power in proportional to the cosine of the angle. In order to produce a constant irradiance on a distant target the total radiation of source and reflection should therefore be proportional to 1/cos² (θ). This yields ##EQU5##

The boundary condition is, in this case, θ=0 at φ=±π/2 because we assume that the strip only radiates on one side, downward. Equation 11 can only be integrated for a α=1:

    sin(φ)=1-|tan(θ)-sin(θ)|.(24)

The acceptance angle function θ as well as the incidence angle for the CEC-type solution are shown in FIG. 8. Integrating yields the reflector shapes plotted in FIG. 9.

The analytical tools described herein can be used to solve real problems which involve reflectors close to the source. This is done by combining the above technique with the edge ray method which has proved so effective in nonimaging designs. That is, the above methods can be applied to edge rays. As a first example, a reflector is designed for a planar, lambertian strip source so as to achieve a predetermined far-field irradiance. The reflector is designed so that the reflected image is immediately adjacent to the source. This is only possible in a negative magnification arrangement. Then the combination of source and its mirror image is bounded by two edge rays as indicated in FIG. 10. The combined angular power density for a source of unit brightness radiated into a certain direction is given by the edge ray separation.

    R sin(2α)=P.sup.o (θ).

By taking the logarithmic derivative of Eq.(25) and substituting the following: ##EQU6##

This describes the right hand side, where θ<0. The other side is the mirror image.

For 2α=π, R diverges just as in the case of the CHC-type solutions for small sources. Thus, in general the full reflector extends to infinity. For practical reasons it will have to be truncated. Let's assume that the reflector is truncated at a point T from which the edge ray is reflected into the direction θτ. For angles θ in between ±θτ the truncation has no effect because the outer parts of the reflector do not contribute radiation in that range. Therefore within this range the truncated reflector also produces strictly the desired illumination. Outside this range the combination of source plus reflector behaves like a flat source bounded by the point T and the opposite edge of the source. Its angular power density is given by Eq.(13) with R=Rτ=constant. The total power Pτ radiated beyond θτ is thus ##EQU7##

In order to produce an intensity P^(o) (θτ) at θτ, R(θτ) must be ##EQU8## The conservation of total energy implies that the truncated reflector radiates the same total power beyond θτ as does the untruncated reflector. ##EQU9##

This equation must hold true for any truncation θ=θτ. It allows us to explicitly calculate α, and with it φ and R, in closed form as functions of θ, if B(θ), that is the integral of P^(o) (θ) is given in closed form. The conservation of total energy also implies that the untruncated reflector radiates the same total power as the bare source. This leads to the normalizing condition. ##EQU10##

This condition may be used to find θ^(max) ; it is equivalent to setting θτ=0, 2ατ=π/2 in Eq.(30). Solving Eq.(30) for α yields. ##EQU11##

Substituting α=(φ-θ)12, yields the acceptance angle function

    φ(θ)=θ=2α.                           (33)

From Eq.(25) the radius is given by ##EQU12##

These equations specify the shape of the reflector in a parametric polar representation for any desired angular power distribution P^(o) (θ). A straight forward calculation shows that Eq. (32) is indeed the solution of the differential equation (27). In fact, Eq.(27) was not needed for this derivation of the reflector shape. We have presented it only to show the consistency of the approach.

For example, to produce a constant irradiance on a plane parallel to the source we must have P^(o) (θ)=1/cos² (θ) and thus B(θ)=cos² (θ)(tan(θ)-tan(θmax)). Using Eq. (31), we find θmax=-π/4 so that B(θ)=cos² (θ)tan(θ)+1 with no undetermined constants.

The resulting acceptance angle function and the reflector profile are shown in FIG. 11 and FIG. 17 respectively. The reflector shape is close to a V-trough. Though, the acceptance angle function is only poorly approximated by a straight fine, which characterizes the V-trough. In FIG. 13 we show the deviation of the reflector shape depicted in FIG. 12 from a true V-trough. Note, that a true V-trough produces a markedly non-constant irradiance distribution proportional to cos(θ+π/4)cos(θ) for 0<-θ<π/4.

As a second example for a specific non-constant irradiance a reflector produces the irradiance distribution on a plane shown in FIG. 14. The corresponding angular power distribution is shown in FIG. 15. The acceptance angle function according to Eq.(33) and (32) and the resulting reflector shape according to Eq.(34) are visualized in FIG. 16 and FIG. 17.

Although the desired irradiance in this example is significantly different from the constant irradiance treated in the example before, the reflector shape again superficially resembles a V-trough and the reflector of the previous example. The subtle difference between the reflector shape of this example and a true V-trough are visualized in FIG. 18 and FIG. 19 where we plot the slope of our reflector and the distance to a true V-trough. Most structure is confined to the region adjacent to the source. The fact that subtle variations in reflector shape have marked effects on the power and irradiance distribution of the device can be attributed to the large incidence angle with which the edge rays strike the outer parts of the reflector.

As mentioned before, in general the reflector is of infinite size. Truncation alters, however, only the distribution in the outer parts. To illustrate the effects of truncation for the reflector of this example, we plot in FIG. 20 the angle up to which the truncated device matches the desired power distribution, as a function of the vertical length of the reflector. Thus for example the truncated device shown in FIG. 17 has the irradiance distribution and power distribution shown in broken line in FIG. 14 and FIG. 15. Note that the reflector truncated to a vertical length of 3 times the source width covers more than 5/6 of the angular range.

B. General Optical Sources

Nonimaging illumination can also be provided by general optical sources provided the geometrical constraints on a reflector can be defined by simultaneously solving a pair of system. The previously recited equations (1) and (2) relate the source angle and angle of light reflection from a reflector surface,

    d/dφ(logR.sub.i)=tan(φ.sub.i -θ.sub.i)/2

and the second general expression of far field illuminance is,

    L(θ.sub.i)·R.sub.i sin(φ.sub.i -θ.sub.i)G(θ.sub.i)=I(θ.sub.i)

where L (θ_(i)) is the characteristic luminance at angle θ_(i) and G (θ_(i)) is a geometrical factor which is a function of the geometry of the light source. In the case of a two dimensional Lambertian light source as illustrated in FIG. 6A, the throughput versus angle for constant illuminance varies as cos² θ. For a three dimensional Lambertian light source shown in FIG. 6D, the throughput versus angle for constant illuminance varies as cos³ θ.

Considering the example of a two dimensional Lamberatian light source and the planar source illustrated in FIG. 6B, the concept of using a general light source to produce a selected far field illurninance can readily be illustrated. Notice with our sign convention angle θ in FIG. 6B is negative. In this example we will solve equations (18) and (19) simultaneously for a uniform far field illuminance using the two dimensional Lambertian source. In this example, equation (19) because,

    R.sub.i sin(φ.sub.i -θ.sub.i)cos.sup.2 θ.sub.i =I(θ.sub.i)

Generally for a bare two dimensional Lambertian source,

    I (θ.sub.i)˜δcos θ.sub.i

    δ˜acos θ.sub.i /l

    l˜d/cos θ

Therefore, I˜cos³ θ.

In the case of selecting a uniform far field illumanance I(θ_(i))=C, and if we solve the equations at the end of the first paragraph of section B.,

d/dφ(log R_(i))=tan (φ_(i) -θ_(i))/2 and

log R_(i) +log sin (φ_(i) -θ_(i))+2 log cos θ_(i) =log C=constant

solving dφ_(i) /dθ_(i) =-2 tan θ_(i) sin (φ_(i) -θ_(i))-cos (φ_(i) -θ_(i))

or let Ψ_(i) =φ_(i) -θ_(i)

dΨ_(i) /dθ_(i) =1+sin Ψ_(i) -2 tan θ_(i) cos Ψ_(i)

Solving numerically by conventional methods, such as the Runge-Kutta method, starting at Ψ_(i) =0 at θ_(i), for the constant illuminance,

dΨ_(i) /dθ_(i) =1+sin Ψ_(i) -n tan θ_(i) cos Ψ_(i) where n is two for the two dimensional source. The resulting reflector profile for the two dimensional solution is shown in FIG. 6C and the tabulated data characteristic of FIG. 6C is shown in Table III. The substantially exact nature of the two dimensional solution is clearly shown in the ray trace fit of FIG. 7A. The computer program used to perform these selective calculation is included as Appendix B of the Specification. For a bare three dimensional Lambertian source where I(θ_(i))˜cos⁴ θ_(i), n is larger than 2 but less than 3.

The ray trace fit for this three dimensional solution is shown in FIG. 7B wherein the "n" value was fitted for desired end result of uniform far field illuminance with the best fit being about n=2.1.

Other general examples for different illuminance sources include,

(1) I(θ_(i))=A exp (Bθ_(i)) for a two dimensional, exponential illuminance for which one must solve the equation,

    dΨ.sub.i /dθ.sub.i =1+sin Ψ.sub.i -2tan θ.sub.i cos Ψ+B

(2) I(θ_(i))=A exp (-Bθ_(i) ² /2) for a two dimensional solution for a Gaussian illuminance for which one must solve,

    dΨ.sub.i /dθ.sub.i =1+sin Ψ.sub.i -2tan θ.sub.i cos Ψ.sub.i -Bθ.sub.i

The equations in the first paragraph of section B can of course be generalized to include any light source for any desired for field illuminance for which one of ordinary skill in the art would be able to obtain convergent solutions in a conventional manner.

A ray trace of the uniform beam profile for the optical device of FIG. 1 is shown in a tabular form of output in Table II below:

                                      TABLE II                                     __________________________________________________________________________     114                                                                               202                                                                               309                                                                               368                                                                               422                                                                               434                                                                               424                                                                               608                                                                               457                                                                               448                                                                               400                                                                               402                                                                               315                                                                               229                                                                               103                                  145                                                                               295                                                                               398                                                                               455                                                                               490                                                                               576                                                                               615                                                                               699                                                                               559                                                                               568                                                                               511                                                                               478                                                                               389                                                                               298                                                                               126                                  153                                                                               334                                                                               386                                                                               465                                                                               515                                                                               572                                                                               552                                                                               622                                                                               597                                                                               571                                                                               540                                                                               479                                                                               396                                                                               306                                                                               190                                  202                                                                               352                                                                               393                                                                               452                                                                               502                                                                               521                                                                               544                                                                               616                                                                               629                                                                               486                                                                               520                                                                               432                                                                               423                                                                               352                                                                               230                                  197                                                                               362                                                                               409                                                                               496                                                                               496                                                                               514                                                                               576                                                                               511                                                                               549                                                                               508                                                                               476                                                                               432                                                                               455                                                                               335                                                                               201                                  241                                                                               377                                                                               419                                                                               438                                                                               489                                                                               480                                                                               557                                                                               567                                                                               494                                                                               474                                                                               482                                                                               459                                                                               421                                                                               379                                                                               230                                  251                                                                               364                                                                               434                                                                               444                                                                               487                                                                               550                                                                               503                                                                               558                                                                               567                                                                               514                                                                               500                                                                               438                                                                               426                                                                               358                                                                               231                                  243                                                                               376                                                                               441                                                                               436                                                                               510                                                                               526                                                                               520                                                                               540                                                                               540                                                                               482                                                                               506                                                                               429                                                                               447                                                                               378                                                                               234                                  233                                                                               389                                                                               452                                                                               430                                                                               489                                                                               519                                                                               541                                                                               547                                                                               517                                                                               500                                                                               476                                                                               427                                                                               442                                                                               344                                                                               230                                  228                                                                               369                                                                               416                                                                               490                                                                               522                                                                               501                                                                               539                                                                               546                                                                               527                                                                               481                                                                               499                                                                               431                                                                               416                                                                               347                                                                               227                                  224                                                                               359                                                                               424                                                                               466                                                                               493                                                                               560                                                                               575                                                                               553                                                                               521                                                                               527                                                                               526                                                                               413                                                                               417                                                                               320                                                                               205                                  181                                                                               378                                                                               392                                                                               489                                                                               485                                                                               504                                                                               603                                                                               583                                                                               563                                                                               530                                                                               512                                                                               422                                                                               358                                                                               308                                                                               194                                  150                                                                               326                                                                               407                                                                               435                                                                               506                                                                               567                                                                               602                                                                               648                                                                               581                                                                               535                                                                               491                                                                               453                                                                               414                                                                               324                                                                               179                                  135                                                                               265                                                                               382                                                                               450                                                                               541                                                                               611                                                                               567                                                                               654                                                                               611                                                                               522                                                                               568                                                                               446                                                                               389                                                                               300                                                                               130                                  129                                                                               213                                                                               295                                                                               364                                                                               396                                                                               404                                                                               420                                                                               557                                                                               469                                                                               435                                                                               447                                                                               351                                                                               287                                                                               206                                                                               146                                  ELEVATION                                                                      __________________________________________________________________________

                  TABLE III                                                        ______________________________________                                         Phi           Theta    r                                                       ______________________________________                                         90.0000       0.000000 1.00526                                                 90.3015       0.298447 1.01061                                                 90.6030       0.593856 1.01604                                                 90.9045       0.886328 1.02156                                                 91.2060       1.17596  1.02717                                                 91.5075       1.46284  1.03286                                                 91.8090       1.74706  1.03865                                                 92.1106       2.02870  1.04453                                                 92.4121       2.30784  1.05050                                                 92.7136       2.58456  1.05657                                                 93.0151       2.85894  1.06273                                                 93.3166       3.13105  1.06899                                                 93.6181       3.40095  1.07536                                                 93.9196       3.66872  1.08182                                                 94.2211       3.93441  1.08840                                                 94.5226       4.19810  1.09507                                                 94.8241       4.45983  1.10186                                                 95.1256       4.71967  1.10876                                                 95.4271       4.97767  1.11576                                                 95.7286       5.23389  1.12289                                                 96.0302       5.48838  1.13013                                                 96.3317       5.74120  1.13749                                                 96.6332       5.99238  1.14497                                                 96.9347       6.24197  1.15258                                                 97.2362       6.49004  1.16031                                                 97.5377       6.73661  1.16817                                                 97.8392       6.98173  1.17617                                                 95.1407       7.22545  1.18430                                                 95.4422       7.46780  1.19256                                                 95.7437       7.70883  1.20097                                                 99.0452       7.94857  1.20952                                                 99.3467       8.18707  1.21822                                                 99.6482       8.42436  1.22707                                                 99.9498       8.66048  1.23607                                                 100.251       8.89545  1.24522                                                 100.553       9.12933  1.25454                                                 100.854       9.36213  1.26402                                                 101.156       9.59390  1.27367                                                 101.457       9.82466  1.28349                                                 101.759       10.0545  1.29349                                                 102.060       10.2833  1.30366                                                 102.362       10.5112  1.31402                                                 102.663       10.7353  1.32457                                                 102.965       10.9645  1.33530                                                 103.266       11.1899  1.34624                                                 103.568       11.4145  1.35738                                                 103.869       11.6383  1.36873                                                 104.171       11.8614  1.38028                                                 104.472       12.0837  1.39206                                                 104.774       12.3054  1.40406                                                 105.075       12.5264  1.41629                                                 105.377       12.7468  1.42875                                                 105.678       12.9665  1.44145                                                 105.980       13.1857  1.45441                                                 106.281       13.4043  1.46761                                                                        1.48108                                                 107.789       14.4898  1.53770                                                 108.090       14.7056  1.55259                                                 108.392       14.9209  1.56778                                                 108.693       15.1359  1.58329                                                 108.995       15.3506  1.59912                                                 109.296       15.5649  1.61529                                                 109.598       15.7788  1.63181                                                 109.899       15.9926  1.64868                                                 110.201       16.2060  1.66591                                                 110.503       16.4192  1.68353                                                 110.804       16.6322  1.70153                                                 111.106       16.8450  1.71994                                                 111.407       17.0576  1.73876                                                 111.709       17.2701  1.75801                                                 112.010       17.4824  1.77770                                                 112.312       17.6946  1.79784                                                 112.613       17.9068  1.81846                                                 112.915       18.1188  1.83956                                                 113.216       18.3309  1.86117                                                 113.518       18.5429  1.88330                                                 113.819       18.7549  1.90596                                                 114.121       18.9670  1.92919                                                 114.422       19.1790  1.95299                                                 114.724       19.3912  1.97738                                                 115.025       19.6034  2.00240                                                 115.327       19.8158  2.02806                                                 115.628       20.0283  2.05438                                                 115.930       20.2410  2.08140                                                 116.231       20.4538  2.10913                                                 116.533       20.6669  2.13761                                                 116.834       20.8802  2.16686                                                 117.136       21.0938  2.19692                                                 117.437       21.3076  2.22782                                                 117.739       21.5218  2.25959                                                 118.040       21.7362  2.29226                                                 118.342       21.9511  2.32588                                                 118.643       22.1663  2.36049                                                 118.945       22.3820  2.39612                                                 119.246       22.5981  2.43283                                                 119.548       22.8146  2.47066                                                 119.849       23.0317  2.50967                                                 120.151       23.2493  2.54989                                                 120.452       23.4674  2.59140                                                 120.754       23.6861  2.63426                                                 121.055       23.9055  2.67852                                                 121.357       24.1255  2.72426                                                 121.658       24.3462  2.77155                                                 121.960       24.5676  2.82046                                                 122.261       24.7898  2.87109                                                 122.563       25.0127  2.92352                                                 122.864       25.2365  2.97785                                                 123.166       25.4611  3.03417                                                 123.467       25.6866  3.09261                                                 123.769       25.9131  3.15328                                                 124.070       26.1406  3.21631                                                 124.372       26.3691  3.28183                                                 124.673       26.5986  3.34999                                                 124.975       26.8293  3.42097                                                 125.276       27.0611  3.49492                                                 125.578       27.2941  3.57205                                                 125.879       27.5284  3.65255                                                 126.181       27.7640  3.73666                                                 126.482       28.0010  3.82462                                                 126.784       28.2394  3.91669                                                 127.085       28.4793  4.01318                                                 127.387       28.7208  4.11439                                                 127.688       28.9638  4.22071                                                 127.990       29.2086  4.33250                                                 128.291       29.4551  4.45022                                                 128.593       29.7034  4.57434                                                 128.894       29.9536  4.70540                                                 129.196       30.2059  4.84400                                                 129.497       30.4602  4.99082                                                 129.799       30.7166  5.14662                                                 130.101       30.9753  5.31223                                                 130.402       31.2365  5.48865                                                 130.704       31.5000  5.67695                                                 131.005       31.7662  5.87841                                                 131.307       32.0351  6.09446                                                 131.608       32.3068  6.32678                                                 131.910       32.5815  6.57729                                                 132.211       32.8593  6.84827                                                 132.513       33.1405  7.14236                                                 132.814       33.4251  7.46272                                                 133.116       33.7133  7.81311                                                 133.417       34.0054  8.19804                                                 133.719       34.3015  8.62303                                                 134.020       34.6019  9.09483                                                 134.322       34.9068  9.62185                                                 134.623       35.2165  10.2147                                                 134.925       35.5314  10.8869                                                 135.226       35.8517  11.6561                                                 135.528       36.1777  12.5458                                                 135.829       36.5100  13.5877                                                 136.131       36.8489  14.8263                                                 136.432       37.1949  16.3258                                                 136.734       37.5486  18.1823                                                 137.035       37.9106  20.5479                                                 137.337       38.2816  23.6778                                                 137.638       38.6625  28.0400                                                 137.940       39.0541  34.5999                                                 138.241       39.4575  45.7493                                                 138.543       39.8741  69.6401                                                 138.844       40.3052  166.255                                                 139.146       40.7528  0.707177E-01                                            139.447       41.2190  0.336171E-01                                            139.749       41.7065  0.231080E-01                                            140.050       42.2188  0.180268E-01                                            140.352       42.7602  0.149969E-01                                            140.653       43.3369  0.129737E-01                                            140.955       43.9570  0.115240E-01                                            141.256       44.6325  0.104348E-01                                            141.558       45.3823  0.958897E-02                                            141.859       46.2390  0.891727E-02                                            142.161       47.2696  0.837711E-02                                            142.462       48.6680  0.794451E-02                                            142.764       50.0816  0.758754E-02                                            143.065       48.3934  0.720659E-02                                            143.367       51.5651  0.692710E-02                                            143.668       51.8064  0.666772E-02                                            143.970       56.1867  0.647559E-02                                            144.271       55.4713  0.628510E-02                                            144.573       54.6692  0.609541E-02                                            144.874       53.7388  0.590526E-02                                            145.176       52.5882  0.571231E-02                                            145.477       50.8865  0.550987E-02                                            145.779       53.2187  0.534145E-02                                            146.080       52.1367  0.517122E-02                                            146.382       50.6650  0.499521E-02                                            146.683       49.5225  0.481649E-02                                            146.985       45.6312  0.459624E-02                                            147.286       56.2858  0.448306E-02                                            147.588       55.8215  0.437190E-02                                            147.889       55.3389  0.426265E-02                                            148.191       54.8358  0.415518E-02                                            148.492       54.3093  0.404938E-02                                            148.794       53.7560  0.394512E-02                                            149.095       53.1715  0.384224E-02                                            149.397       52.5498  0.374057E-02                                            149.698       51.8829  0.363992E-02                                            150.000       51.1597  0.354001E-02                                            ______________________________________                                    

C. Extended, Finite Size Sources

In this section we demonstrate how compact CEC-type reflectors can be designed to produce a desired irradiance distribution on a given target space from a given, finite size, source. The method is based on tailoring the reflector to a family of edge-rays, but at the same time the edge rays of the reflected source image are also controlled.

In order to tailor edge rays in two dimensions, for example, one can assume a family of edge rays, such as are produced by a luminaire source. Through each point in the space outside the luminaire source there is precisely one edge ray. The direction of the edge rays is a continuous and differentiable (vector) function of position. If we have a second, tentative family of edge-rays represented by another continuous vector function in the same region of space, we can design a reflector which precisely reflects one family onto the other. Each point in space is the intersection of precisely one member of each family. Therefore, the inclination of the desired reflector in each point in space can be calculated in a conventional, well known manner. Thus, one can derive a differential equation which uniquely specifies the reflector once the starting point is chosen.

We can, for example, formalize this idea for the case where the tentative family of edge rays is given only along a reference line which is not necessarily a straight line. This pertains to the usual problems encountered in solving illumination requirements.

Referring to FIG. 21, let a=a(x) be the two dimensional unit vector 100 pointing towards the edge of a source 102 as seen from a point x, where k=k(t) is a parametrization of reference line 104 according to a scalar parameter t. Let u(t) be a unit vector 106 pointing in the direction of an edge ray 107 desired at the reference location specified by t. We can parametrize the contour of a reflector 108 with respect to the reference line 104 by writing the points on the reflector 108 as:

    R(t)=k(t)+Du(t)                                            (35)

Here the scalar D denotes the distance from a point on the reference line 104 to the reflector 108 along the desired edge ray 107 through this point.

Designing the shape of the reflector 108 in this notation is equivalent to specifying the scalar function D=D(t). An equation for D is derived from the condition that the reflector 108 should reflect the desired edge ray 107 along u(t) into the actual edge ray a(R(t)) and vice versa: ##EQU13## Inserting Eq. (35) from above yields: ##EQU14##

Here the dots indicate scalar products. Equation (37) is a scalar differential equation for the scalar function D(t). By solving this equation, we can determine the reflector 108 which tailors the desired family of the edge ray 107 specified by the unit vector, u, 106 to the source 102 characterized by the vector function, a.

This approach can also be used to tailor one family of the edge rays 107 onto another with refractive materials rather then reflectors. Equation (36) then is replaced by Snell's law.

Consequently, the condition for the existence of a solution in this embodiment is that each point on the reflector 108 is intersected by precisely one member of the family of tentative edge rays. To be able to define this family of edge rays 107 along the reference line 104, each point on the reference line 104 must also be intersected by precisely one tentative edge ray. This is less than the requirement that the tentative edge rays define a physical surface which produces them. The family of the edge rays 107 of a physical contour (for example right edge rays) must also satisfy the further requirement that precisely one edge ray passes through each point of the entire space exterior to the contour. Indeed we can produce families of such edge rays by tailoring, but which cannot be produced by a single physical source. This is confirmed by observations that curved mirrors produce not only a distorted image of the source, but furthermore an image is produced that appears to move as the observer moves.

The condition that each point on the reflector 108, as well as each point on the reference line 104, should be intersected by precisely one of the desired edge rays 107 implies that the caustic formed by these edge rays 107 cannot intersect the reflector 108 or the reference line 104. The caustic must therefore either be entirely confined to the region between the reflector 108 and the reference line 104, or lie entirely outside this region. The first of these alternatives characterizes the CEC-type solutions, while the second one defines CHC-type solutions.

In order to determine the desired edge rays 107, the irradiance, for example, from a Lambertian source of uniform brightness B is given by its projected solid angle, or view factor. In a conventional, known manner the view factor is calculated by projecting the source 102 first on a unit sphere surrounding the observer (this yields the solid angle) and then projecting the source 102 again onto the unit circle tangent to the reference plane. The view factor is determined by the contour of the source 102 as seen by the observer. In two dimensions for example, the irradiance E is,

    E=B(sin r.sub.R -sin r.sub.L)                              (38)

where r_(R) and R_(L) are the angles between the normal to the reference line and the right and left edge rays striking the observer, respectively. If we know the brightness B, the desired irradiance E and one edge ray, then Eq. (38) can be used to determine the desired direction of the other edge ray.

Consider the example of a source 110 of given shape (see FIG. 22). We then know the direction of the edge rays as seen by an observer as a function of the location of the observer. The shape of the source 110 can be defined by all its tangents. We can now design the reflector 108 so that it reflects a specified irradiance distribution onto the given reference line 104 iteratively.

In this iterative process if an observer proceeds, for example, from right to left along reference line 112, the perceived reflection moves in the opposite direction for a CEC-type solution. As shown in FIG. 22A a right edge ray 114 as seen by the observer, is the reflection of the right edge, as seen from reflector 116, and further plays the role of leading edge ray 114' along the reflector 116. A left edge ray 118 is just trailing behind, and this is shown in FIG. 22A as reflected trailing edge ray 118'. For a CHC-type reflector 126 (see FIG. 22B) the reflected image of the source 110 moves in the same direction as the observer, and the right edge as seen by the observer is the reflection of the left edge. If part of the reflector 126 is known, then a trailing edge ray 128' which has been reflected by the known part of the reflector 126, can be calculated as a function of location on the reference line 112. Equation (38) consequently specifies the direction of leading edge ray 130. Then, Eq. (37) can be solved to tailor the next part of the reflector profile to this leading edge ray 130.

Considering the boundary conditions, if the reflector 116 or 126 is terminated, then the reflected radiation does not terminate where the leading edge from the end of the reflector 116 or 126 strikes the reference line 112. Rather the reflected radiation ends where the trailing edge from the end of the reflector 116 or 126 strikes the reference line 112 (see FIG. 23). Thus, there is a `decay` zone 131 on the reference line 112 which subtends an equal angle at the source 110 as seen from the end of the reflector 116 or 126. In this region the previously leading edge is at an end location 129 of the reflector 116 or 126, while the trailing edge gradually closes in. An analogous `rise` zone 132 exists at the other end of the reflector 116, 126, where the trailing edge is initially fixed to a `start` position 134 of the reflector 116. However, there is an important conceptual difference between these two regions, in that the `rise` of the irradiance can be modeled by tailoring the reflector 116, 126 to the leading edge, while the `decay` cannot be influenced once the reflector 116, 126 is terminated. Therefore, there is a difference in which way we can proceed in the iterative tailoring of the reflector 116, 126.

If the source 110 radiates in all directions and we want to avoid trapped radiation (that is radiation reflected back onto the source 110), then the reflected radiation from each side of the reflector 140 should cover the whole target domain of the reflector 140 (see FIG. 24). At the same time, the normal to the reflector surface should not intersect the source 110. Therefore, left and right side portions 142 and 143, respectively, of the reflectors 140 are joined in a cusp. An observer in the target domain thus perceives radiation from two distinct reflections of the source 110, one in each of the portions 142 and 143 of the reflector 140, in addition to the direct radiation from the source 110.

If we assume symmetry as shown in FIG. 24 and that the reflector 140 is preferred to be continuous and differentiable (except for the cusp in the symmetry plane), then we require that as seen from the symmetry plane, the two perceived reflections are equal. For all other points in the target domain we now have the additional degree of freedom of choosing the relative contributions of each of the portions 142 and 143 of the reflector 140. In CEC-type solutions both reflections appear to be situated between the target space and the reflector 140. Thus, as the observer moves, both reflection images move in the opposite direction. To that end, when the observer approaches the outermost part of the illuminated target region, the reflection on the same side first disappears at the cusp in the center. Thereafter, the reflection opposite to the observer starts to disappear past the outer edge of the opposite reflector, while the source itself is shaded by the outer edge of the other reflector portion on the observer side. These events determine the end point of the reflector 140 because now the total radiation in the target region equals the total radiation emitted by the source 110.

CEC-Type Reflector for Constant Irradiance

A CEC-type reflector 150 can produce a constant irradiance on a distant plane from a finite size cylindric source 152 of uniform brightness. This requires the angular power distribution to be proportional to 1/cos² (θ). In FIG. 25 we show the necessary power from both reflections so that the total power is as required. The reflector 150 is depicted in FIG. 26. The reflector 150 is designed starting from cusp 154 in the symmetry axes. Note that each reflection irradiates mostly the opposite side, but is visible from the same side too. Some angles have been particularly designated by the letters A through and E in FIG. 25. The corresponding edge rays are indicated also in FIG. 27.

Between -A and A angles the reflections are immediately adjacent to the source 152. The cusp 154 in the center is not visible. Between A and B angles the reflection from the same side as the observer slowly disappears at the cusp 154, while the other increases in size for compensation. Starting with C the source 152 is gradually eclipsed by the end of the reflector 150. The largest angle for which a constant irradiance can be achieved is labeled D. The source 152 is not visible. The power is produced exclusively by the opposite side reflection. The reflector 150 is truncated so that between D and E the reflection gradually disappears at the end of the reflector 150.

The inner part of the reflector 150 which irradiates the same side, is somewhat arbitrary. In the example shown, we have designed it as an involute because this avoids trapped radiation and at the same time yields the most compact design. At the center the power from each reflection is very nearly equal to that of the source 152 itself. Once the power radiated to the same side is determined, the reflector 150 is designed so that the sum of the contributions of the two reflections and the source 152 matches the desired distribution. Proceeding outward, the eclipsing of the source 152 by the reflector 150 is not known at first, because it depends on the end point. This problem is solved by iterating the whole design procedure several times.

The point of truncation is determined by the criterium that the reflector 150 intersects the edge rays marked B from the cusp 154. This is because the preferred design is based on a maximum of one reflection. This criterium is also the reason for designing the inner part as an involute.

The angular decay range D to E in FIGS. 25 and 27 depends only on the distance of the end point to the source 152. Depending on the starting distance from the cusp 154 to the source 152, the device can be designed either more compact, but with a broader decay zone, or larger, and with a more narrow decay zone. The reflector 150 shown has a cusp distance of 2.85 source diameters. The end point is at a distance of 8.5 source diameters. This ensures that a constant irradiance is produced between -43 and 43 degrees. The decay zone is only 7 degrees. This design was chosen in order that the source 152 is eclipsed just before the angle of truncation.

The reflector 150 cannot be made much more compact as long as one designs for a minimum of one reflection. At the angle D the opening is nearly totally filled with radiation as seen in FIG. 27. The distance the reflector 150 extends downward from the source 152 is also determined by the maximum power required to produce at angle D. The distance of the cusp 154 also cannot be diminished, otherwise the criterium for the end of the reflection 150 is reached sooner, the reflector 150 has to be truncated and the maximum power produced is also less.

The embodiments described hereinbefore involve at most one reflection. However, in other forms of the invention various systems based on multiple reflections can be designed using the teachings provided herein. As more reflections contribute, the freedom of the designer increases. This freedom can be used to adapt the reflector to other criteria, such as a need for compactness. In any case, independent of the number of reflections, once the general architecture has been determined, tailoring the reflector to one set of edge rays determines its shape without the need for approximations or a need to undergo optimizations. 

We claim:
 1. A method of manufacturing a collector of light of irradiance I from a radiant source, comprising the steps of:providing a transducer device for collecting the light; and providing a light reflecting surface by constructing a reflector contour with a family of edge rays defined along a reference line defined by k(t) and forming a shape for said reflector contour relative to said reference line by tracing a vector R(t) to form said shape where t is a scalar parameter position and wherein:

    R(t)=k(t)+Du(t)

where k(t)=a parameterization of said reference line;D=a distance from a point on said reference line to said reflecting surface along a desired edge ray through the point; n=unit vector along a desired direction of said desired edge ray; with said reflector contour reflecting said desired edge ray into actual edge ray a(R(t)), where a is a multidimensional unit vector pointing towards an edge of said radiant light, and said D being the solutions of:

    dD/dt=((dk(t)/dt)·(a-u)+D(du/dt)·a)/1-a·u


2. 2. The method as defined in claim 1 further including the step of providing light refractive medium means characteristic of a dielectric for generating the family of edge rays.
 3. The method as defined in claim 1 futher including the step of defining an edge ray having undergone multiple reflections.
 4. The method as defined in claim 1 further including light refracting medium means and including the additional step of tailoring the desired edge ray into the actual edge ray.
 5. The method as defined in claim 1 wherein said reflector contour is comprised of at least two reflector contours.
 6. The method as defined in claim 5 wherein said two reflector contours comprise include a cusp positioned therebetween.
 7. The method as defined in claim 6 wherein said two reflector contours comprise a mirror image surface disposed about said cusp.
 8. The method as defined in claim 1 wherein said reflector contour is comprised of a compound concentrator reflector.
 9. The method as defined in claim 8 wherein said compound concentrator reflector is selected from the group consisting of CHC, CEC and CPC.
 10. The method as defined in claim 1 further including the step of defining said reflector contour by generating tangent lines to a surface of the contour, said tangent lines generating a trailing edge ray which is used in conjunction with a function describing the irradiance, I, to calculate a leading edge ray.
 11. The method as defined in claim 1 wherein the expression dD/dt is used in conjunction with calculating the leading edge ray to determine a new portion of the reflector contour.
 12. A method of collecting light of irradiance I from a radiant source over an angular range, comprising the steps of:collecting light from the source using a transducer means; and defining light means for manipulating light received from the source using at least one of the steps (a) using light refracting medium means and (b) using a light reflector contour having a reflective surface established by the step of defining a family of edge rays relative to a reference line expressed as k(t) and a point located on said reference line and further defined by a desired edge ray passing through the point and extending to said reflector contour, wherein t is a scalar parameter position and defining said reflector contour by applying an expression R(t):

    R(t)=k(t)+Du(t)

wherek(t)=a parameterization of said reference line; D=a distance from the point on said reference line to at least one of said refracting medium means and said reflecting surface along said desired edge ray through the point; u=a unit vector along a desired direction of said desired edge ray; and said reflector contour and said light refracting medium means reflecting and refracting, respectively, said desired edge ray into an actual edge ray a R(t)), where a is a multidimensional unit vector pointing towards an edge of said transducer means and wherein the desired edge ray is tailored into the actual edge ray by at least one of said reflector contour and said retracting medium means.
 13. The method as defined in claim 12 further including the step of defining an edge ray having undergone multiple reflections.
 14. The method as defined in claim 12 further including light refracting medium means and including the additional step of tailoring the desired edge ray into the actual edge ray.
 15. The method as defined in claim 12 wherein said reflector contour comprises at least two reflector contours.
 16. The method as defined in claim 15 wherein said two reflector contours include a cusp positioned therebetween.
 17. The method as defined in claim 16 wherein said two reflector contours comprise a mirror image surface disposed about said cusp.
 18. The method as defined in claim 12 wherein said reflector contour comprises a compound concentrator reflector.
 19. The method as defined in claim 18 wherein said compound concentrator reflector is selected from the group consisting of CHC. CEC and CPC.
 20. The method as defined in claim 12 further including the step of defining said reflector contour by generating tangent lines to a surface of the reflector contour, said tangent lines generating a trailing edge ray which is used in conjunction with a function describing the irradiance, I, to calculate a leading edge ray.
 21. The method as defined claim 20 wherein the expression dD/dt is used in conjunction with calculating the leading edge ray to determine a new portion of the reflector contour. 